Synthetic aperture multi-telescope tracker apparatus

Claim 1

A synthetic aperture multi-telescope tracker apparatus comprising in combination: a plurality of telescopes each providing an output signal, a beam splitter in optical alignment with each of said plurality of telescopes to receive an output signal therefrom, said beam splitter providing a plurality of output signals which correspond respectively to the received output signal from each of said plurality of telescopes, a plurality of photo-detector units to respectively receive one output signal of said plurality of output signals from said beam splitter, each photo-detector unit of said plurality of photo-detector units respectively providing an x error and a y error signal corresponding to the tilt error of said plurality of telescopes, a chopper unit in optical alignment with said beam splitter to receive each output signal from said plurality of telescopes, said chopper unit generating a timing pulse, said chopper unit sequentially sampling each output signal to provide a plurality of sampled telescope return signals, a photo-detector means to receive each signal of said plurality of sampled telescope return signals and provide a plurality of x-y error signals corresponding thereto, a timing generator to receive said timing pulses from said chopper unit, said timing generator providing timing signals corresponding to said timing pulses, a plurality of integrator/low pass filter units to respectively receive said x error and y error signals from said plurality of photo-detector units, each of said plurality of integrator/low pass filter units integrating its error signal over a predetermined interval and filtering its error signal to provide the D.C. component of the telescope tilt error, a plurality of sample and hold units connected respectively to said plurality of integrator/low pass filter units to receive therefrom the D.C. component of the telescope tilt error, said plurality of sample and hold units sampling and holding said D.C. ccmponent of the telescope tilt error to provide a D.C. tilt error signal, a plurality of complementary low pass filter units to respectively receive said D.C. tilt error signal from said plurality of sample and hold units, a plurality of complementary high pass filter units to respectively receive said x error and y error signal from said plurality of photo-detector units, said plurality of ccmplementary high pass filter units respectively filtering said x error and y error signal to provide the A.C. component of the telescope tilt error, each of said plurality of complementary high pass filter units respectively providing an A.C. tilt error signal, said plurality of complementary high pass filter units are respectively matched to said plurality of complementary low pass filter units so that they selectively pass a portion of the frequency spectrum but are matched so that the transfer function of their sum is unity at all frequencies, and, a plurality of summing units respectively connected to said plurality of complementary high pass filter units and said plurality of complementary low pass filter units such that the output signals of the corresponding filter units in x error signals and y error signals are combined to provide a tilt error signal in x and y for each of said plurality of telescopes.